English

Second-order perturbation theory: the problem of infinite mode coupling

General Relativity and Quantum Cosmology 2016-11-15 v1

Abstract

Second-order self-force computations, which will be essential in modeling extreme-mass-ratio inspirals, involve two major new difficulties that were not present at first order. One is the problem of large scales, discussed in [Phys. Rev. D 92, 104047 (2015)]. Here we discuss the second difficulty, which occurs instead on small scales: if we expand the field equations in spherical harmonics, then because the first-order field contains a singularity, we require an arbitrarily large number of first-order modes to accurately compute even a single second-order mode. This is a generic feature of nonlinear field equations containing singularities, allowing us to study it in the simple context of a scalar toy model in flat space. Using that model, we illustrate the problem and demonstrate a robust strategy for overcoming it.

Keywords

Cite

@article{arxiv.1608.06783,
  title  = {Second-order perturbation theory: the problem of infinite mode coupling},
  author = {Jeremy Miller and Barry Wardell and Adam Pound},
  journal= {arXiv preprint arXiv:1608.06783},
  year   = {2016}
}

Comments

18 pages, 6 figures, submitted to PRD

R2 v1 2026-06-22T15:29:08.733Z